Two types of supernova remnant are morphologically recognized; shell
type and center filled. As outlined in the VERITAS proposal the full
array should detect 20 Galactic supernova remnants within 4 kpc
of the Earth if the diffusive shock emission models are indeed
correct. Table 5 lists the top 20 candidate targets of VERITAS
with both a shell and center filled morphology.
Name | RA | DEC | Size | Morphology
![]() |
(hr min) | (deg min) | (arcmin) | ||
W44 | 18h 53![]() |
1![]() ![]() |
35x27 | S |
W51 | 19h 21![]() |
14![]() ![]() |
30 | S |
Cygnus Loop | 20h 49![]() |
30![]() ![]() |
230x160 | S |
gamma Cygni | 20h 19![]() |
40![]() ![]() |
60 | S |
W63 | 20h 17![]() |
45![]() ![]() |
95x65 | S |
HB21 | 20h 43![]() |
50![]() ![]() |
120x90 | S |
CAS A | 23h 21![]() |
58![]() ![]() |
5 | S |
Tycho | 0h 22![]() |
63![]() ![]() |
8 | S |
G156.2+5.7 | 4h 54![]() |
51![]() ![]() |
110 | S |
IC443 | 6h 14![]() |
22![]() ![]() |
45 | S |
W28 | 17h 57![]() |
-23![]() ![]() |
42 | C |
SN AD386 | 18h 8![]() |
-19![]() ![]() |
4 | C |
G21.5-0.9 | 18h 30![]() |
-10![]() ![]() |
1.2 | F |
KES 75 | 18h 43![]() |
-3![]() ![]() |
3 | C |
G32.1-0.9 | 18h 50![]() |
-1![]() ![]() |
40 | C |
G54.1+0.3 | 19h 28![]() |
18![]() ![]() |
1.5 | F |
CTB 80 | 19h 51![]() |
32![]() ![]() |
80 | * |
CTB 87 | 20h 14![]() |
37![]() ![]() |
8x6 | F |
CTA 1 | 0h 4![]() |
72![]() ![]() |
90 | S |
3C58 | 2h 1![]() |
64![]() ![]() |
9x5 | F |
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